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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/766
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dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2006-03-14T10:12:28Z-
dc.date.available2006-03-14T10:12:28Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 159-165en
dc.identifier.urihttp://hdl.handle.net/2248/766-
dc.description.abstractThe existence of cool regions where dust can condense is explored in RCB stars at minimumen
dc.format.extent217897 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectRCB starsen
dc.subjectdust condensationen
dc.subjectC2 moleculeen
dc.titleProbing circumstellar dust formation through high resolution spectroscopyen
dc.typeArticleen
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